The Fate of the Universe
Will the Universe
continue to expand at such a hurried pace? Will the expansion teeter out,
or will the Universe collapse back in on itself under the pull of gravity? These are the big questions about the fate of the Universe that MAP hopes to answer.
The fate of the Universe depends on its contents: how much matter
and energy there is. If there is a lot of matter, then gravity will dominate,
slowly reigning in the expansion and pulling all matter together back to
one point. Some call this the Big Crunch. If there is not so much matter
but rather dark energy -- that force that acts like anti-gravity -- then
the Universe will continue to expand until ever single speck of matter is
pulled infinitely apart from each other.
Both scenarios sound scary,
but neither would happen for trillions upon trillions of years. A more pleasant
notion is the situation where the Universe has just the right about of matter
and dark energy to keep it from flying apart or crashing in.
MAP will measure the ratio of ordinary matter, dark matter and dark energy. Scientists refer to the density of matter as omega () and the contribution of dark energy as the cosmological constant, denoted by lambda (). Knowing lambda and omega will provide a hint of what's in store for the next 10100 years. Will life still exist? It will be difficult, to say the least. If the Universe continues to expand, stars will all but disappear after 1014 years. And protons are thought to decay after 1050
years. It is hard to think about life without protons. That's 100 trillion
trillion trillion trillion years or, in less scientific terms, a real long